Probing a muonic force with the periastron advance in binary pulsar systems

TL;DR

This paper uses precise measurements of periastron advance in binary pulsar systems to set new, stringent constraints on ultralight muonic mediators, surpassing previous gravitational wave limits.

Contribution

It introduces a novel method to constrain ultralight muonic mediators using binary pulsar data, accounting for muon abundance and long-range force effects.

Findings

Periastron advance provides sensitive constraints on muonic mediators.

Constraints reach muonic couplings as small as 10^{-21}.

Limits surpass LIGO/Virgo gravitational wave bounds by about an order of magnitude.

Abstract

Pulsars, highly magnetized, rotating neutron stars, can have significant muon abundances in their dense cores, making them promising environments to probe ultralight mediators coupled to muons. The precise measurement of periastron advance in binary pulsar systems provides a sensitive probe of such long-range forces. In this work, we study the periastron advance constraints from binary pulsar systems on the ultralight muonic mediators. We compute the muon number fraction in neutron stars, by properly taking into account the suppression effect of the long-range muonic force. We find that the periastron advance constraints impose the most stringent constraints on ultralight muonic mediators in the mass range of $\simeq(10^{-17},\,2\times10^{-15})$ eV, probing muonic couplings as small as $\mathcal{O}(10^{-21})$, which surpass the limits from LIGO/Virgo gravitational wave measurements, by about an order of magnitude.